Interactive scientific tool for exploring how noise affects weak signals and how smoothing can help recover hidden patterns.
This project simulates a clean scientific signal, adds random noise, and then applies smoothing to show how hidden patterns can be recovered.
Users can explore:
Noise is unavoidable in real scientific measurements.
In astronomy and instrumentation, weak signals are often affected by:
Understanding signal-to-noise ratio is essential for interpreting data from telescopes, spectrographs, detectors, and laboratory instruments.
A weak signal can be hidden beneath random fluctuations.
Smoothing can help reveal the underlying pattern, but excessive smoothing may remove real features.
Instruments often record both real signal and unwanted noise.
A simplified signal-to-noise ratio can be written as:
```text SNR = signal strength / noise strength
In this project:
signal strength is estimated from the spread of the true signal noise strength is estimated from the spread of the random noise
This is a simplified educational model. Real scientific instruments may include more complex noise sources.
See RESEARCH_QUALITY.md for the validation layer, reference anchors, equations and research boundaries added to this repository.